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[vsnet-campaign-sn 585] SN observation from IAUC 8097 (bright SN 2003cg)

SN2003cg  20030313.3  <190:C  KAI
SN2003cg  20030321.51  144:C  KIt
SN2003cg  20030322.3   149:C  KAI
SN2003cg  20030322.444 143:C  KIt
SN2003cg  20030322.559 155:C  KuR
SN2003cg  20030322.835 145:C  ARB

# SN 2003cg (10:14:15.97, +3:28:02.5 (J2000.0), offset = 14"E, 5"N) is
# hosted by NGC 3169, a nearby spiral (SA(s)a pec) galaxy.  The
# expected maximum for typical SN Ia is mag about 12.8 (!).  NGC 3169
# has produced SN IIL 1984L, whose maximum was B=15.2.

SN2003ch  20030310.2  <190:C  KAI
SN2003ch  20030321.2   174:C  KAI
SN2003ch  20030322.2   170:C  KAI

# SN 2003ch (7:17:57.92, +9:41:34.9 (J2000.0), offset = 5"E, 13"N) is
# hosted by UGC 3787, an elliptical (or lenticular) galaxy which is a
# western component of the galaxy pair.  There are a log of foreground
# stars, so the identification should be done carefully.

SN2003ci  20030305.4  <190:C  KAI
SN2003ci  20030321.4   175:C  KAI
SN2003ci  20030322.4   175:C  KAI

# SN 2003ci (11:10:23.83, +4:49:35.9 (J2000.0), offset = 11"W, 12"S)
# is hosted by UGC 6212, a disturbed spiral galaxy interacting with
# the southern smaller one.  The new object is superimposed on the
# southern arm.  There is a foreground star also superimposed on the
# disk, so the careful identification would be needed.  The expected
# maximum for typicaol SN Ia is comparable with the discovery
# magnitude. 

Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan

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